Flare Observed by a Dozen Instruments

Nugget
Number:	230
1st Author:	Lucia Kleint
2nd Author:	Kevin Reardon
Published:	July 14, 2014
Next Nugget:	TBD
Previous Nugget:	RHESSI is Annealing Now

Introduction

We live in a golden age for research on solar flares, observationally speaking. This statement reflects not only the existence of powerful satellite observatories (RHESSI, Hinode, SDO, Fermi, STEREO, and now IRIS, as well as basic standbys such as GOES), but also advanced ground-based instrumentation at observatories such as the powerful Arcetri/NSO IBIS instrument. limited of course by observatory longitudes and the resulting day/night problem. In addition many spacecraft also observe the interplanetary consequences of a solar eruption. Count the instruments up and one quickly exceeds a dozen; these instruments individually mostly have unique capabilities and people cheerfully write papers about their particular individual discoveries. Put them all together and one has a wonderful opportunity to gain a broad insight into flare development, if fortune smiles and many actually have suitable coverage.

Just about that situation happened on March 29, 2014, when SOL2014-03-29 (X1.0) occurred; see the SDO movies.

All of the observatories listed above got some data, mostly with good coverage and with correct pointing. A high-resolution observatory can often miss a big flare simply by staring at the wrong spot. For general reference we offer Figure 1, showing the basic GOES time history.

Figure 1: Three different views of the basic time-series soft X-ray data for the flare, from NOAA's GOES. The plots show the flux (blue), its time derivative (red and gold), and a blow-up of four minutes in the impulsive phase. The left panel is a standard log-scaled plot, and the right two are more direct linear scalings. The sign of the time derivative is reversed (the gold) where it turns negative. Note the presence of impulsive-phase pulsations and likely oscillatory variations in the gradual phase.

What's really new

The newest participant is the IRIS spacecraft, the first really to target the "interface region" bridging the gap between the hot surface of the Sun (the photosphere) and the very hot corona.

Conclusions

It often happens that a major flare happens and everybody in the community scrambles to write a "gee whiz" paper about the particularly noteworthy thing their instrument has seen. Often, of course, they include as much data from other sources as possible, and of course they work hard at drawing physically meaningful conclusions. Nevertheless they tend to work simultaneously and not necessarily in a coordinated way, and what appears in the literature may be disorganized as a result. Only seldom does the community do a retrospective look at a given well-observed event, but we recommend that here because of the excellent coverage.

References

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